MathWorks Shack-Hartmann Modeling
Subaperture spot migration, wavefront slope and wavefront reconstruction steps
Verification date: 2026-10-24
View original public information →Facing the microlens array element, using the separation point array comparison as the observation route, the focus number, center and point distance are planned to be output. The page is for project evaluation and does not mean that the development has been completed or has been accepted on site.
Separate and numberable multiple light spots, fixed receiving plane and field of view. Microlens array, reference spot field and wavefront calibration components
Separate and numberable multiple light spots, fixed receiving plane and field of view
Existing algorithmic evidence:A101–A112 only complete analytical synthesis spot and controlled geometry verification; see laser_spot_benchmark.json
The light point detection front-end or timing statistics module can be reused, but the project still needs to add geometric calibration, time synchronization, motion compensation or equipment system integration.
Gaps in this scenario:Point sequence numbering, local ROI, crosstalk and occlusion processing are required; A108 only matches by distance in the same coordinate system. Single aperture focal length requires axial scanning. The existing code provides center extraction, and the wavefront slope and reconstruction core need to be added.
Route-level gaps:Point sequence numbering, local ROI, crosstalk and occlusion processing are required; A108 only matches by distance in the same coordinate system
"Partially reusable" only describes the relative development volume and does not constitute a commitment to accuracy, tempo, stability or delivery time.
Verify point counts, match rates, and mismatches using known lattice and artificial defect/overlap/scrambling data. Comparison with known aberration elements and interferometers
| Acceptance items | Evidence required for project confirmation | Current status |
|---|---|---|
| Inputs and samples | Real device original frames, normal/abnormal samples, exposure and light path conditions, sample grouping and set aside | Not provided, waiting for project input |
| Magnitude and Error | Independent reference value, calibration record, error statistical caliber and mutual confirmation threshold | Not verified |
| Exceptions and boundaries | Anticipated handling of missed detections, false detections, overexposure, occlusion, reflection, out-of-view and communication abnormalities | To be defined |
| System integration | Interface, time synchronization, deployment platform, tempo, log, version and continuous running record | Not integrated |
The source supports measurement principles or similar applications; the module combination, device and acceptance method in this scenario are engineering derivation, and product verification has not been completed.
Subaperture spot migration, wavefront slope and wavefront reconstruction steps
Verification date: 2026-10-24
View original public information →Light point correlation, missing points, and wavefront reconstruction constraints
Verification date: 2026-10-24
View original public information →Array focus loss and misalignment inspection
Please describe the task object, original picture or video, target indicators, device platform, interface and sample situation.
Phone: 13910119357